Electron Dissipation and Electromagnetic Work
Date
2024-10-14
Journal Title
Journal ISSN
Volume Title
Publisher
JGR: Space Physics
Abstract
With the increase in technical capabilities of computer simulation in recent years, it has become feasible to quantify the degradation of fluid scale plasma and electromagnetic energies in favor of increases of internal energies. While it is understood that electromagnetic energy can be exchanged with fluid scale velocities, it is the pressure strain interaction that exchanges energy between fluid motions and internal energy. Here using simulations of both turbulence and reconnection we show that for electrons, the pressure strain and electromagnetic work are closely related and are frequently comparable when appropriate time and spatial averaging is applied. Otherwise, the instantaneous spatial averaged pressure strain and electromagnetic work are nearly equal for slowly evolving systems, like the reconnection case, while they differ significantly in rapidly evolving systems, like the turbulence case. This clarifies the relationship between these two quantities, which are each frequently used as measures of dissipation.
Key Points
- Time integrated volume averaged electromagnetic work does not formally or generally correspond to dissipation
- Due to small electron mass, time integrated volume averaged pressure strain and electromagnetic work are nearly equal for electrons
- Differences between instantaneous electromagnetic work and pressure strain can be considerable, but for electrons, these average to zero
Plain Language Summary
The electromagnetic field changes the fluid velocity of each type of plasma particle. Meanwhile, the pressure of each plasma species, interacts with nonuniform fluid velocities to produce heat. The intermediate steps are in general, complicated, but because electrons are so light, a special simplifying approximation holds, equating properly averaged electromagnetic work on electrons to the rate of increase of electron internal energy. This result may help clarify differences in how the reconnection and turbulence communities quantify “dissipation”.
Description
This article was originally published in JGR: Space Physics. The version of record is available at: https://doi.org/10.1029/2024JA033105.
© 2024. American Geophysical Union. All Rights Reserved.
This article will be embargoed until 04/14/2025.
Keywords
energy dissipation, electromagnetic work, pressure strain interaction, plasma turbulence, magnetic reconnection
Citation
Yang, Y., Adhikari, S., & Matthaeus, W. H. (2024). Electron dissipation and electromagnetic work. Journal of Geophysical Research: Space Physics, 129, e2024JA033105. https://doi.org/10.1029/2024JA033105